Brillouin–Wigner perturbation theory
E33422
Brillouin–Wigner perturbation theory is a formulation of quantum mechanical perturbation theory that uses an energy-dependent effective Hamiltonian to obtain improved approximations to eigenvalues and eigenstates.
Aliases (2)
Statements (41)
| Predicate | Object |
|---|---|
| instanceOf |
perturbation theory
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quantum mechanical formalism → |
| advantage |
can improve convergence of perturbation series in some problems
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| aimsTo |
obtain improved approximations to eigenstates
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obtain improved approximations to eigenvalues → |
| appliedIn |
nuclear shell-model calculations
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| appliesTo |
discrete spectra
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time-independent Hamiltonians → |
| assumes |
existence of a solvable unperturbed Hamiltonian
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|
| basedOn |
partition of Hamiltonian into unperturbed and perturbation parts
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|
| category |
approximation method in quantum theory
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|
| characteristic |
energy appearing on both sides of the eigenvalue equation
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| comparedTo |
Rayleigh–Schrödinger perturbation theory
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| contrastWith |
Rayleigh–Schrödinger perturbation theory using energy-independent effective Hamiltonian
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| developedIn |
20th century
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| feature |
nonlinear dependence of energy corrections on the exact energy
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| field |
quantum mechanics
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| focusesOn |
corrections to eigenvalues and eigenvectors of the unperturbed Hamiltonian
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| formalismType |
time-independent perturbation theory
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| framework |
Hilbert space of quantum states
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| goal |
improve accuracy beyond low-order perturbation results
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| involves |
projection operators onto model space and complementary space
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| limitation |
leads to implicit equations for energies
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requires self-consistent solution for eigenvalues → |
| mathematicalForm |
series expansion in powers of the perturbation
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|
| namedAfter |
Eugene Wigner
→
Léon Brillouin → |
| relatedConcept |
Brillouin–Wigner expansion
→
quasi-degenerate perturbation theory → |
| relatedTo |
Feshbach projection formalism
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effective Hamiltonian methods → |
| requires |
choice of model space
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definition of projection operators → |
| usedFor |
bound-state problems in quantum mechanics
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many-body quantum systems → |
| usedIn |
atomic physics
→
condensed matter physics → molecular physics → |
| usedToDerive |
effective interactions in model spaces
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|
| uses |
energy-dependent effective Hamiltonian
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|
| yields |
energy-dependent effective Hamiltonian in model space
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|
Referenced by (3)
| Subject (surface form when different) | Predicate |
|---|---|
|
Brillouin–Wigner perturbation theory
("quasi-degenerate perturbation theory")
→
Brillouin–Wigner perturbation theory ("Brillouin–Wigner expansion") → |
relatedConcept |
|
Rayleigh–Schrödinger perturbation theory
→
|
relatedTo |